Table 2.
Stellar parameters, spectrophotometric distances, color excesses, and photospheric mass fractions of the two program stars.
| Object | M | τ | log(L/L⊙) | R⋆ | d | E(B − V) | X | Y | Z | ||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (Myr) | (R⊙) | (pc) | (mag) | |||||||||||||||||||||||
| PG 1610+062 | 4.4 |
 |
83 |
 |
2.66 |
 |
3.3 |
 |
17 300 |
 |
0.024 |
 |
0.635 |
 |
0.344 |
 |
0.021 |
 |
|||||||||
| HD 137366 | 5.1 |
 |
83 |
 |
2.99 |
 |
4.7 |
 |
360 |
 |
0.056 |
 |
0.667 |
 |
0.316 |
 |
0.016 |
 |
|||||||||
Notes. Except for the distance d, for which photometric uncertainties are included in the error budget, uncertainties cover only the effects induced by variations of 2% in Teff and 0.1 in log(g) and are formally taken to be 99% confidence limits (see Irrgang et al. 2014 for details).
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